A Multiepoch X-Ray Study of the Nearby Seyfert 2 Galaxy NGC 7479: Linking Column Density Variability to the Torus Geometry
An Early-time Optical and Ultraviolet Excess in the Type-Ic SN 2020oi
Digging a little deeper: characterizing three new extreme ULX candidates
Dust in the central parsecs of unobscured AGN: more challenges to the torus
Hubble Space Telescope Imaging Reveals That SN 2015bh Is Much Fainter than Its Progenitor
Nothing to see here: failed supernovae are faint or rare
Photometric and spectroscopic evolution of the interacting transient AT 2016jbu(Gaia16cfr)
Progenitor, environment, and modelling of the interacting transient AT 2016jbu (Gaia16cfr)
SN 2019ehk: A Double-peaked Ca-rich Transient with Luminous X-Ray Emission and Shock-ionized Spectral Features
The Blue Supergiant Progenitor of the Supernova Imposter AT 2019krl
The changing-type SN 2014C may come from an 11-M star stripped by binary interaction and violent eruption
The impact of satellite trails on Hubble Space Telescope observations
The nature of the symbiotic candidate 2MASS J07363415+6538548 in the field of NGC 2403
The Type II supernova SN 2020jfo in M 61, implications for progenitor system, and explosion dynamics
TRGB Distances to Galaxies Based on Hubble Space Telescope (HST) Images in One F814W Filter1
Ultraluminous X-ray sources in seven edge-on spiral galaxies
Instrument
ACS/WFC
Temporal Coverage
2019-03-25T06:37:22Z/2019-09-28T20:51:48Z
Version
1.0
Mission Description
Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
European Space Agency, Sand comma David J., 2020, 'The Identification of Failed Supernovae', 1.0, European Space Agency, https://doi.org/10.5270/esa-ba9tse3